Parabolic Jets from the Spinning Black Hole in M87

23 Oct 2018 Nakamura Masanori Asada Keiichi Hada Kazuhiro Pu Hung-Yi Noble Scott Tseng Chihyin Toma Kenji Kino Motoki Nagai Hiroshi Takahashi Kazuya Algaba Juan-Carlos Orienti Monica Akiyama Kazunori Doi Akihiro Giovannini Gabriele Giroletti Marcello Honma Mareki Koyama Shoko Lico Rocco Niinuma Kotaro Tazaki Fumie

The M87 jet is extensively examined by utilizing general relativistic magnetohydrodynamic (GRMHD) simulations as well as the steady axisymmetric force-free electrodynamic (FFE) solution. Quasi-steady funnel jets are obtained in GRMHD simulations up to the scale of $\sim 100$ gravitational radius ($r_{\rm g}$) for various black hole (BH) spins... (read more)

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Categories


  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • ASTROPHYSICS OF GALAXIES
  • FLUID DYNAMICS
  • PLASMA PHYSICS